SDO HMI 2014-11-03 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.82 | 0.00 | 9.45 | -20.10 | 78.76 | -24.11 | 136.79 | 0.5602 | 637.9 | 539.8 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 0.94 | -20.83 | 85.38 | -17.49 | 146.16 | 0.5065 | 969.0 | 784.2 | |
| 0.00 | 1.30 | 0.00 | 0.72 | -16.87 | 84.76 | -18.11 | 140.05 | 0.4652 | 774.0 | 671.9 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -20.11 | 81.67 | -21.20 | 140.09 | 0.5314 | 381.0 | 348.6 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -20.34 | 79.09 | -23.78 | 137.23 | 0.5588 | 719.0 | 522.5 | |
| 0.00 | 1.90 | 0.00 | 1.14 | -20.51 | 78.96 | -23.91 | 137.29 | 0.5618 | 734.0 | 601.6 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -20.44 | 78.06 | -24.80 | 136.18 | 0.5699 | 644.0 | 554.6 | |
| 0.00 | 2.33 | 0.00 | 1.41 | -20.25 | 77.68 | -25.19 | 135.51 | 0.5720 | 483.0 | 367.7 | |
| 0.00 | 0.69 | 0.00 | 0.42 | -20.08 | 77.04 | -25.83 | 134.59 | 0.5768 | 747.0 | 521.0 | |
| 0.00 | 2.08 | 0.00 | 1.26 | -20.16 | 76.49 | -26.37 | 134.12 | 0.5831 | 702.0 | 661.7 | |
| 0.00 | 1.30 | 0.00 | 0.79 | -19.82 | 75.92 | -26.95 | 133.08 | 0.5860 | 687.0 | 542.7 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -20.61 | 75.70 | -27.17 | 133.89 | 0.5953 | 350.0 | 445.3 | |
| 0.00 | 1.30 | 0.00 | 0.80 | -20.82 | 75.37 | -27.50 | 133.83 | 0.6005 | 465.0 | 338.8 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |